NASA Confirms Liquid Lake On Saturn Moon

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July 30, 2008

Dwayne Brown 
NASA Headquarters, Washington                          
202-358-1726 
dwayne.c.brown@xxxxxxxx 

Carolina Martinez 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-9382 
carolina.martinez@xxxxxxxxxxxx 

Lori Stiles 
University of Arizona, Tucson 
520-360-0574 
lstiles@xxxxxxxxxxxxx                 
RELEASE: 08-193

NASA CONFIRMS LIQUID LAKE ON SATURN MOON

PASADENA, Calif. -- NASA scientists have concluded that at least one 
of the large lakes observed on Saturn's moon Titan contains liquid 
hydrocarbons, and have positively identified the presence of ethane. 
This makes Titan the only body in our solar system beyond Earth known 
to have liquid on its surface. 

Scientists made the discovery using data from an instrument aboard the 
Cassini spacecraft. The instrument identified chemically different 
materials based on the way they absorb and reflect infrared light. 
Before Cassini, scientists thought Titan would have global oceans of 
methane, ethane and other light hydrocarbons. More than 40 close 
flybys of Titan by Cassini show no such global oceans exist, but 
hundreds of dark lake-like features are present. Until now, it was 
not known whether these features were liquid or simply dark, solid 
material. 

"This is the first observation that really pins down that Titan has a 
surface lake filled with liquid," said Bob Brown of the University of 
Arizona, Tucson. Brown is the team leader of Cassini's visual and 
mapping instrument. The results will be published in the July 31 
issue of the journal Nature. 

Ethane and several other simple hydrocarbons have been identified in 
Titan's atmosphere, which consists of 95 percent nitrogen, with 
methane making up the other 5 percent. Ethane and other hydrocarbons 
are products from atmospheric chemistry caused by the breakdown of 
methane by sunlight. 

Some of the hydrocarbons react further and form fine aerosol 
particles. All of these things in Titan's atmosphere make detecting 
and identifying materials on the surface difficult, because these 
particles form a ubiquitous hydrocarbon haze that hinders the view. 
Liquid ethane was identified using a technique that removed the 
interference from the atmospheric hydrocarbons. 

The visual and mapping instrument observed a lake, Ontario Lacus, in 
Titan's south polar region during a close Cassini flyby in December 
2007. The lake is roughly 7,800 square miles in area, slightly larger 
than North America's Lake Ontario. 

"Detection of liquid ethane confirms a long-held idea that lakes and 
seas filled with methane and ethane exist on Titan," said Larry 
Soderblom, a Cassini interdisciplinary scientist with the U.S. 
Geological Survey in Flagstaff, Ariz. "The fact we could detect the 
ethane spectral signatures of the lake even when it was so dimly 
illuminated, and at a slanted viewing path through Titan's 
atmosphere, raises expectations for exciting future lake discoveries 
by our instrument." 

The ethane is in a liquid solution with methane, other hydrocarbons 
and nitrogen. At Titan's surface temperatures, approximately 300 
degrees Fahrenheit below zero, these substances can exist as both 
liquid and gas. Titan shows overwhelming evidence of evaporation, 
rain, and fluid-carved channels draining into what, in this case, is 
a liquid hydrocarbon lake. 

Earth has a hydrological cycle based on water and Titan has a cycle 
based on methane. Scientists ruled out the presence of water ice, 
ammonia, ammonia hydrate and carbon dioxide in Ontario Lacus. The 
observations also suggest the lake is evaporating. It is ringed by a 
dark beach, where the black lake merges with the bright shoreline. 
Cassini also observed a shelf and beach being exposed as the lake 
evaporates. 

"During the next few years, the vast array of lakes and seas on 
Titan's north pole mapped with Cassini's radar instrument will emerge 
from polar darkness into sunlight, giving the infrared instrument 
rich opportunities to watch for seasonal changes of Titan's lakes," 
Soderblom said. 

Launched in Oct. 1997, Cassini's 12 instruments have returned a daily 
stream of data from Saturn's system. The mission is a cooperative 
project of NASA, the European Space Agency and the Italian Space 
Agency. 

For information on Cassini, visit: 










http://www.nasa.gov/cassini 

	
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